BEGIN:VCALENDAR VERSION:2.0 PRODID:-//Plone.org//NONSGML plone.app.event//EN X-WR-TIMEZONE:Europe/Paris BEGIN:VEVENT SUMMARY:CEMP Stars as Probes of First-Star Nucleosynthesis\, the IMF\, and Galactic Assembly (Working Group Meeting). (9-13 September\, Geneve\, Swi tzerland) DTSTART;VALUE=DATE:20190909 DTEND;VALUE=DATE:20190914 DTSTAMP;VALUE=DATE-TIME:20201230T131445Z UID:6a054df06c814837afde39afce5da7dd ATTENDEE;CN="Aldo Mura-Guzman The Australian National University ";ROLE= REQ-PARTICIPANT:Aldo Mura-Guzman The Australian National University ATTENDEE;CN="André Maeder Geneva Observatory ";ROLE=REQ-PARTICIPANT:And ré Maeder Geneva Observatory ATTENDEE;CN="Anish Amarsi Max Planck Institute for Astronomy ";ROLE=REQ- PARTICIPANT:Anish Amarsi Max Planck Institute for Astronomy ATTENDEE;CN="Anke Arentsen Leibniz-Institut für Astrophysik Potsdam ";R OLE=REQ-PARTICIPANT:Anke Arentsen Leibniz-Institut für Astrophysik Pots dam ATTENDEE;CN="Anne Verhamme anne.verhamme@unige.ch ";ROLE=REQ-PARTICIPANT :Anne Verhamme anne.verhamme@unige.ch ATTENDEE;CN=;ROLE=REQ-PARTICIPANT: ATTENDEE;CN="Arthur Choplin Konan University ";ROLE=REQ-PARTICIPANT:Arth ur Choplin Konan University ATTENDEE;CN="Arūnas Kučinskas Vilnius University, Lithuania ";ROLE=REQ -PARTICIPANT:Arūnas Kučinskas Vilnius University, Lithuania ATTENDEE;CN="Asa Skuladottir MPIA, Heidelberg ";ROLE=REQ-PARTICIPANT:Asa Skuladottir MPIA, Heidelberg ATTENDEE;CN="Avrajit Bandyopadhyay Indian Institute of Astrophysics, Ban galore ";ROLE=REQ-PARTICIPANT:Avrajit Bandyopadhyay Indian Institute of Astrophysics, Bangalore ATTENDEE;CN="Beatriz Barbuy Universidade de São Paulo ";ROLE=REQ-PARTIC IPANT:Beatriz Barbuy Universidade de São Paulo ATTENDEE;CN="Bing Du ";ROLE=REQ-PARTICIPANT:Bing Du ATTENDEE;CN="Birgitta Nordstrom Niels Bohr Institute, Copenhagen Univers ity, Denmark ";ROLE=REQ-PARTICIPANT:Birgitta Nordstrom Niels Bohr Instit ute, Copenhagen University, Denmark ATTENDEE;CN="Camilla Juul Hansen MPIA ";ROLE=REQ-PARTICIPANT:Camilla Juu l Hansen MPIA ATTENDEE;CN="Chiaki Kobayashi University of Hertfordshire ";ROLE=REQ-PAR TICIPANT:Chiaki Kobayashi University of Hertfordshire ATTENDEE;CN="Cristina Chiappini Leibniz Institute for Astrophysics Potsd am - AIP ";ROLE=REQ-PARTICIPANT:Cristina Chiappini Leibniz Institute for Astrophysics Potsdam - AIP ATTENDEE;CN="David Aguado University of Cambridge ";ROLE=REQ-PARTICIPANT :David Aguado University of Cambridge ATTENDEE;CN="David Yong Australian National University ";ROLE=REQ-PARTIC IPANT:David Yong Australian National University ATTENDEE;CN="Devin Whitten University of Notre Dame ";ROLE=REQ-PARTICIPA NT:Devin Whitten University of Notre Dame ATTENDEE;CN="Dogus Ozuyar Ankara University ";ROLE=REQ-PARTICIPANT:Dogus Ozuyar Ankara University ATTENDEE;CN="Else Starkenburg Leibniz Institute for Astrophysics Potsdam ";ROLE=REQ-PARTICIPANT:Else Starkenburg Leibniz Institute for Astrophys ics Potsdam ATTENDEE;CN="Falk Herwig University of Victoria ";ROLE=REQ-PARTICIPANT:F alk Herwig University of Victoria ATTENDEE;CN="Federico Sestito Observatoire Astronomique de Strasbourg "; ROLE=REQ-PARTICIPANT:Federico Sestito Observatoire Astronomique de Stras bourg ATTENDEE;CN="Friedrich Thielemann University of Basel and GSI Darmstadt ";ROLE=REQ-PARTICIPANT:Friedrich Thielemann University of Basel and GSI Darmstadt ATTENDEE;CN="Gabriele Cescutti I.N.A.F. Osservatorio Astronomico di Trie ste ";ROLE=REQ-PARTICIPANT:Gabriele Cescutti I.N.A.F. Osservatorio Astro nomico di Trieste ATTENDEE;CN="Gaël Buldgen University of Geneva ";ROLE=REQ-PARTICIPANT:G aël Buldgen University of Geneva ATTENDEE;CN="Georges Meynet Université de Genève ";ROLE=REQ-PARTICIPAN T:Georges Meynet Université de Genève ATTENDEE;CN="Jiannan Zhang NAOC ";ROLE=REQ-PARTICIPANT:Jiannan Zhang N AOC ATTENDEE;CN="Jinmi Yoon University of Notre Dame ";ROLE=REQ-PARTICIPANT: Jinmi Yoon University of Notre Dame ATTENDEE;CN="John Wise Georgia Institute of Technology ";ROLE=REQ-PARTIC IPANT:John Wise Georgia Institute of Technology ATTENDEE;CN="Joseph Zepeda University of Notre Dames ";ROLE=REQ-PARTICIP ANT:Joseph Zepeda University of Notre Dames ATTENDEE;CN="Kaitlin Rasmussen University of Notre Dame ";ROLE=REQ-PARTI CIPANT:Kaitlin Rasmussen University of Notre Dame ATTENDEE;CN="Krishna Choudhury University of Calcutta ";ROLE=REQ-PARTICI PANT:Krishna Choudhury University of Calcutta ATTENDEE;CN="kwame appiah ghana atomic energy commission ";ROLE=REQ-PART ICIPANT:kwame appiah ghana atomic energy commission ATTENDEE;CN="Laura Murphy Trinity College Dublin ";ROLE=REQ-PARTICIPANT: Laura Murphy Trinity College Dublin ATTENDEE;CN="Leah Cox ";ROLE=REQ-PARTICIPANT:Leah Cox ATTENDEE;CN="Lionel Haemmerlé Université de Genève ";ROLE=REQ-PARTICI PANT:Lionel Haemmerlé Université de Genève ATTENDEE;CN="Mahavir Sharma ICRAR, Curtin University ";ROLE=REQ-PARTICIP ANT:Mahavir Sharma ICRAR, Curtin University ATTENDEE;CN="Mattis Magg Insitute for Theoretical Astrophysics, Universi ty of Heidelberg ";ROLE=REQ-PARTICIPANT:Mattis Magg Insitute for Theoret ical Astrophysics, University of Heidelberg ATTENDEE;CN="Mohammad Mardini National Astronomical Observatories of Chi na ";ROLE=REQ-PARTICIPANT:Mohammad Mardini National Astronomical Observa tories of China ATTENDEE;CN="Myoungwon Jeon Kyung Hee University ";ROLE=REQ-PARTICIPANT: Myoungwon Jeon Kyung Hee University ATTENDEE;CN="Nial Tanvir University of Leicester ";ROLE=REQ-PARTICIPANT: Nial Tanvir University of Leicester ATTENDEE;CN="Ondrea Clarkson University of Victoria ";ROLE=REQ-PARTICIPA NT:Ondrea Clarkson University of Victoria ATTENDEE;CN="Piercarlo Bonifacio GEPI, Observatoire de Paris, PSL, CNRS ";ROLE=REQ-PARTICIPANT:Piercarlo Bonifacio GEPI, Observatoire de Paris, PSL, CNRS ATTENDEE;CN="Piyush Sharda Australian National University ";ROLE=REQ-PAR TICIPANT:Piyush Sharda Australian National University ATTENDEE;CN="Rana Ezzeddine Massachusetts Institute of Technology ";ROLE =REQ-PARTICIPANT:Rana Ezzeddine Massachusetts Institute of Technology ATTENDEE;CN="Raphael Hirschi Keele University ";ROLE=REQ-PARTICIPANT:Rap hael Hirschi Keele University ATTENDEE;CN="Roberto Gallino University of Torino(Italy) ";ROLE=REQ-PART ICIPANT:Roberto Gallino University of Torino(Italy) ATTENDEE;CN="Romain Lucchesi EPFL Laboratoire d'astrophysique, ESO ";ROL E=REQ-PARTICIPANT:Romain Lucchesi EPFL Laboratoire d'astrophysique, ESO ATTENDEE;CN="Sarah Dietz University of Notre Dame ";ROLE=REQ-PARTICIPANT :Sarah Dietz University of Notre Dame ATTENDEE;CN="Shingo Hirano Kyushu University ";ROLE=REQ-PARTICIPANT:Shin go Hirano Kyushu University ATTENDEE;CN="Silvia Rossi Universidade de São Paulo/IAG ";ROLE=REQ-PART ICIPANT:Silvia Rossi Universidade de São Paulo/IAG ATTENDEE;CN="stefania salvadori Florence University, Physics and Astrono my Department ";ROLE=REQ-PARTICIPANT:stefania salvadori Florence Univers ity, Physics and Astronomy Department ATTENDEE;CN="Susmitha Rani Antony Tata Institute of Fundamental Research , Mumbai, India ";ROLE=REQ-PARTICIPANT:Susmitha Rani Antony Tata Institu te of Fundamental Research, Mumbai, India ATTENDEE;CN="Sutirtha Sengupta Department of Applied Mathematics, UC San ta Cruz ";ROLE=REQ-PARTICIPANT:Sutirtha Sengupta Department of Applied M athematics, UC Santa Cruz ATTENDEE;CN="Sylvia Ekström Geneva University ";ROLE=REQ-PARTICIPANT:Sy lvia Ekström Geneva University ATTENDEE;CN="Sébastien Martinet University of Geneva ";ROLE=REQ-PARTICI PANT:Sébastien Martinet University of Geneva ATTENDEE;CN="Tadafumi Matsuno NAOJ/SOKENDAI ";ROLE=REQ-PARTICIPANT:Tadaf umi Matsuno NAOJ/SOKENDAI ATTENDEE;CN="Tejpreet Kaur Panjab University, Chandigarh ";ROLE=REQ-PART ICIPANT:Tejpreet Kaur Panjab University, Chandigarh ATTENDEE;CN="Theodora Xylakis-Dornbusch ZAH/LSW University of Heidelberg ";ROLE=REQ-PARTICIPANT:Theodora Xylakis-Dornbusch ZAH/LSW University of Heidelberg ATTENDEE;CN="Thomas Nordlander Australian National University ";ROLE=REQ -PARTICIPANT:Thomas Nordlander Australian National University ATTENDEE;CN="Tilman Hartwig University of Tokyo ";ROLE=REQ-PARTICIPANT:T ilman Hartwig University of Tokyo ATTENDEE;CN="Timothy Beers University of Notre Dame ";ROLE=REQ-PARTICIPA NT:Timothy Beers University of Notre Dame ATTENDEE;CN="Vanessa Hill UCA, Observatoire de la Côte d'Azur, CNRS, La boratoire Lagrange ";ROLE=REQ-PARTICIPANT:Vanessa Hill UCA, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange ATTENDEE;CN="Vinicius Placco University of Notre Dame ";ROLE=REQ-PARTICI PANT:Vinicius Placco University of Notre Dame ATTENDEE;CN="Volker Bromm University of Texas at Austin ";ROLE=REQ-PARTI CIPANT:Volker Bromm University of Texas at Austin ATTENDEE;CN="Wei-Ting Liao University of Illinois at Urbana-Champaign "; ROLE=REQ-PARTICIPANT:Wei-Ting Liao University of Illinois at Urbana-Cham paign ATTENDEE;CN="Zhen Yuan Shanghai Astronomical Observatory ";ROLE=REQ-PART ICIPANT:Zhen Yuan Shanghai Astronomical Observatory ATTENDEE;CN="Şeyma Çalışkan Ankara University";ROLE=REQ-PARTICIPANT: Şeyma Çalışkan Ankara University ATTENDEE;CN=;ROLE=REQ-PARTICIPANT: CONTACT:Georges Meynet and Timothy Beers\, +41 22 379 23 98\, georges.meyn et@unige.ch / tbeers@nd.edu\, https://indico.cern.ch/event/791509/overvi ew CREATED;VALUE=DATE-TIME:20190611T160456Z DESCRIPTION:The beginning of the stellar era in the Universe is a singular ly fascinating phase in the history of the Cosmos. The baryonic material f illing the Universe at that time\, having a composition inherited from Big Bang nucleosynthesis\, has its physical characteristics modified by the v ery first stars. Indeed\, the first stars will change the degree of ionize d material in their vicinity\, and\, through their winds and/or supernova explosion\, will inject energy\, momentum\, and newly-synthesized elements . Some pockets of gas\, enriched by the first stars\, will in turn form ne w stars\, whose initial composition is inherited from the first nucleosynt hetic events. These low-mass stars can live sufficiently long to be observ ed today in halo of the Galaxy\, providing the opportunity to obtain infor mation about the very high redshift Universe by the study of nearby stars. How did these processes happen? How were these processes different from similar ones occurring in the present Universe? What can they teach us ab out the infancy of the Universe during the reionization era? These are the questions that will be discussed during this workshop\, questions that ar e particularly topical at a time when new facilities\, such as SKA\, JWST\ , and the next generation of extremely large telescopes have as one of the ir prime objectives to probe this very period. At present\, observation al constraints on these first stars are scarce and/or indirect. Important constraints come from observations of the elemental abundances of very\, e xtremely\, and ultra iron-poor stars that likely formed from the ejecta of the first stellar generations. Of course the full story can be complex\, as some elements might be formed by more than one source\, and others may be somewhat altered by in-situ processes that occurred in the star that is observed today. Nevertheless\, through the accumulation of observational data\, progress made in numerical simulations\, and in our deeper understa nding of the physical processes involved\, a much more complete and detail ed story can be told. LAST-MODIFIED;VALUE=DATE-TIME:20200128T164843Z LOCATION:Geneva University\, 30 quai Ernest Ansermet in Auditorium A100 Sc iences II URL:http://www.chetec.eu/events/cemp-stars-as-probes-of-first-star-nucleos ynthesis-the-imf-and-galactic-assembly-working-group-meeting END:VEVENT END:VCALENDAR